Modelling the atmosphere of potential habitable planets

Autor(en)
Nicolas Iro
Abstrakt

The list of planets discovered in the habitable zone of its star is continuously growing. We present a simple one-dimension radiative transfer model in order to better infer on the habitability of such systems. Particular focus is on the TRAPPIST-1 planets (Gillon et al.2017), particularly on planets b, c, d, e and f.

Organisation(en)
Institut für Astrophysik
Journal
Proceedings of the International Astronomical Union
Band
14
Seiten
172-175
Anzahl der Seiten
4
DOI
https://doi.org/10.1017/S1743921319002874
Publikationsdatum
01-2020
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
Schlagwörter
ASJC Scopus Sachgebiete
Public Health, Environmental and Occupational Health, Astronomy and Astrophysics, Nutrition and Dietetics, Medicine (miscellaneous), Space and Planetary Science
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/aaf0e252-c128-4a5a-bbc8-a723379aabf5